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BzK selection<br />
ALMA deep field: predicted properties of UDF galaxies<br />
continuum: observed UV/optical SEDs → SED models (Da Cunha) → dust<br />
luminosity (from <strong>at</strong>tenu<strong>at</strong>ion in UV) → FIR luminosity → ALMA flux densities<br />
lines: LFIR → LCO (Daddi et al., Genzel et al.), assuming range of CO excit<strong>at</strong>ions MW⟷M82)<br />
Band 6<br />
Band 7<br />
Band 3<br />
Whole sample (13,099 galaxies)<br />
0.0 ≤ z < 1.5 (5,660 galaxies)<br />
1.5 ≤ z < 2.5 (4,286 galaxies)<br />
2.5 ≤ z < 5.0 (3,153 galaxies)
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